Neutron stars, supernova explosions and the transition to quark matter

Details Neutron stars, supernova explosions and the transition to quark matter Neutron stars, supernova explosions and the transition to quark matter

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999nupha.661..633d&link_type=abstract

Nuclear Physics A, Volume 661, Issue 1-4, p. 633-636.

Physics

Nuclear Physics

2

Scientific paper

The structure of a hybrid star is discussed using both the MIT bag model
and the Color Dielectric Model to describe the quark matter phase. A
finite temperature equation of state is introduced to discuss the
possibility that the transition to quark matter takes place during the
pre-supernova collapse.

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